[MOK2016b] HSC J120859.23-020034.8 , the SIMBAD biblio

[MOK2016b] HSC J120859.23-020034.8 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:42:07

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2018ApJ...869..150M 17       D               1 111 151 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar luminosity function and contribution to cosmic reionization at z = 6. MATSUOKA Y., STRAUSS M.A., KASHIKAWA N., et al.
2018PASJ...70S..35M 17       D               1 66 104 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8. MATSUOKA Y., ONOUE M., KASHIKAWA N., et al.
2019ApJ...880...77O 794       D     X C       19 13 89 Subaru high-z exploration of low-luminosity quasars (SHELLQs). VI. Black hole mass Measurements of six quasars at 6.1 <= z <= 6.7. ONOUE M., KASHIKAWA N., MATSUOKA Y., et al.
2019MNRAS.490.2542P viz 16       D               1 2245 ~ Unveiling the weak radio quasar population at z≥4. PERGER K., FREY S., GABANYI K.E., et al.
2019PASJ...71..111I 710       D     X C       17 16 53 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). VIII. A less biased view of the early co-evolution of black holes and host galaxies. IZUMI T., ONOUE M., MATSUOKA Y., et al.
2020MNRAS.494..789R viz 16       D               1 489 25 The near and mid-infrared photometric properties of known redshift z >= 5 quasars. ROSS N.P. and CROSS N.J.G.
2020ApJ...903...60I 469       D     X         12 39 13 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity zone analysis for faint quasar spectra at z ∼ 6. ISHIMOTO R., KASHIKAWA N., ONOUE M., et al.
2020ApJ...905...51S viz 83             C       1 42 62 The X-SHOOTER/ALMA sample of quasars in the epoch of reionization. I. NIR spectral modeling, iron enrichment, and broad emission line properties. SCHINDLER J.-T., FARINA E.P., BANADOS E., et al.
2021ApJ...908..124L 17       D               1 38 28 Constraining the quasar radio-loud fraction at z ∼ 6 with deep radio observations. LIU Y., WANG R., MOMJIAN E., et al.
2021ApJ...914L..26F 20       D               1 10 33 Seeding supermassive black holes with self-interacting dark matter: a unified scenario with baryons. FENG W.-X., YU H.-B. and ZHONG Y.-M.
2021A&A...656A.137G viz 17       D               1 493 12 Low frequency radio properties of the z > 5 quasar population. GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al.
2022ApJ...927..237I 47           X         1 4 19 Rapid Growth of Seed Black Holes during Early Bulge Formation. INAYOSHI K., NAKATANI R., TOYOUCHI D., et al.
2022MNRAS.517.1264L 102       D         F     2 94 3 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) - XV. Constraining the cosmic reionization at 5.5 < z < 7. LU T.-Y., GOTO T., HASHIMOTO T., et al.
2022ApJ...941..106F viz 17       D               1 120 26 The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. FARINA E.P., SCHINDLER J.-T., WALTER F., et al.
2023ApJ...954..164T 17       D               1 106 ~ Modeling the Central Supermassive Black Hole Mass of Quasars via the LSTM Approach. TABASI S.S., SALMANI R.V., KHALILIYAN P., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024MNRAS.534.2062V 287       D     X C F     5 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., et al.
2025MNRAS.536.3177A 19       D               1 93 ~ Deciphering the origins and growth of supermassive black holes. AGGARWAL Y.
2025ApJ...979..183I 19       D               1 73 ~ Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XXI. Candidate Red Quasars at z ≥ 6 from Near-infrared Photometry. IWAMOTO R., MATSUOKA Y., IMANISHI M., et al.

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